Weak interaction strengths for supernovae calculations via the (t,3He) reaction on medium-heavy nuclei

R.G.T. Zegers; A.L. Cole; H. Akimune; S.M. Austin; D. Bazin; A.M. van den Berg; G.P.A. Berg; J Brown; I. Daito; Y. Fujita; M. Fujiwara; K. Hara; M.N. Harakeh; G.W. Hitt; M. Howard; J. Jänecke; T. Kawabata; T. Nakamura; H. Ueno; G Schatz; B.M. Sherrill; M. Steiner

doi:10.1016/j.nuclphysa.2005.05.018

Weak interaction strengths for supernovae calculations via the (t,3He) reaction on medium-heavy nuclei

R.G.T. Zegers, A.L. Cole, H. Akimune, S.M. Austin, D. Bazin, A.M. van den Berg, G.P.A. Berg, J Brown, I. Daito, Y. Fujita, M. Fujiwara, K. Hara, M.N. Harakeh, G.W. Hitt, M. Howard, J. Jänecke, T. Kawabata, T. Nakamura, H. Ueno, G SchatzB.M. Sherrill, M. Steiner

Research output: Contribution to journal › Article › Academic › peer-review

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Abstract

The Ni-58 (t, He-3)Co-58 reaction at 112 MeV/nucleon was measured to identify strength associated with Gamow-Teller transitions in the T-z = +1 direction. The experiment is a test case for future similar studies. The main aim of such studies is to test theoretical models used to predict Gamow-Teller strength distributions that serve as input for supernovae evolution calculations. The results indicate that the (t, He-3) reaction is indeed a powerful tool to perform such tests.

Original language	English
Pages (from-to)	67C-70C
Number of pages	4
Journal	Nuclear Physics A
Volume	758
DOIs	https://doi.org/10.1016/j.nuclphysa.2005.05.018
Publication status	Published - 25-Jul-2005
Event	8th International Symposium on Nucle in the Cosmos (NIC8) - Vancouver, Canada Duration: 19-Jul-2004 → 23-Jul-2004

Keywords

CHARGE-EXCHANGE REACTIONS
SHELL-MODEL CALCULATIONS
MASS RANGE A=45-65
INTERACTION RATES
DISTRIBUTIONS
COLLAPSE

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Zegers, R. G. T., Cole, A. L., Akimune, H., Austin, S. M., Bazin, D., van den Berg, A. M., Berg, G. P. A., Brown, J., Daito, I., Fujita, Y., Fujiwara, M., Hara, K., Harakeh, M. N., Hitt, G. W., Howard, M., Jänecke, J., Kawabata, T., Nakamura, T., Ueno, H., ... Steiner, M. (2005). Weak interaction strengths for supernovae calculations via the (t,3He) reaction on medium-heavy nuclei. Nuclear Physics A, 758, 67C-70C. https://doi.org/10.1016/j.nuclphysa.2005.05.018

@article{9f7fc7ce88844bce89d55274e601dc19,

title = "Weak interaction strengths for supernovae calculations via the (t,3He) reaction on medium-heavy nuclei",

abstract = "The Ni-58 (t, He-3)Co-58 reaction at 112 MeV/nucleon was measured to identify strength associated with Gamow-Teller transitions in the T-z = +1 direction. The experiment is a test case for future similar studies. The main aim of such studies is to test theoretical models used to predict Gamow-Teller strength distributions that serve as input for supernovae evolution calculations. The results indicate that the (t, He-3) reaction is indeed a powerful tool to perform such tests.",

keywords = "CHARGE-EXCHANGE REACTIONS, SHELL-MODEL CALCULATIONS, MASS RANGE A=45-65, INTERACTION RATES, DISTRIBUTIONS, COLLAPSE",

author = "R.G.T. Zegers and A.L. Cole and H. Akimune and S.M. Austin and D. Bazin and {van den Berg}, A.M. and G.P.A. Berg and J Brown and I. Daito and Y. Fujita and M. Fujiwara and K. Hara and M.N. Harakeh and G.W. Hitt and M. Howard and J. J{\"a}necke and T. Kawabata and T. Nakamura and H. Ueno and G Schatz and B.M. Sherrill and M. Steiner",

year = "2005",

month = jul,

day = "25",

doi = "10.1016/j.nuclphysa.2005.05.018",

language = "English",

volume = "758",

pages = "67C--70C",

journal = "Nuclear Physics A",

publisher = "ELSEVIER SCIENCE BV",

note = "8th International Symposium on Nucle in the Cosmos (NIC8) ; Conference date: 19-07-2004 Through 23-07-2004",

}

Zegers, RGT, Cole, AL, Akimune, H, Austin, SM, Bazin, D, van den Berg, AM, Berg, GPA, Brown, J, Daito, I, Fujita, Y, Fujiwara, M, Hara, K, Harakeh, MN, Hitt, GW, Howard, M, Jänecke, J, Kawabata, T, Nakamura, T, Ueno, H, Schatz, G, Sherrill, BM & Steiner, M 2005, 'Weak interaction strengths for supernovae calculations via the (t,3He) reaction on medium-heavy nuclei', Nuclear Physics A, vol. 758, pp. 67C-70C. https://doi.org/10.1016/j.nuclphysa.2005.05.018

TY - JOUR

T1 - Weak interaction strengths for supernovae calculations via the (t,3He) reaction on medium-heavy nuclei

AU - Zegers, R.G.T.

AU - Cole, A.L.

AU - Akimune, H.

AU - Austin, S.M.

AU - Bazin, D.

AU - van den Berg, A.M.

AU - Berg, G.P.A.

AU - Brown, J

AU - Daito, I.

AU - Fujita, Y.

AU - Fujiwara, M.

AU - Hara, K.

AU - Harakeh, M.N.

AU - Hitt, G.W.

AU - Howard, M.

AU - Jänecke, J.

AU - Kawabata, T.

AU - Nakamura, T.

AU - Ueno, H.

AU - Schatz, G

AU - Sherrill, B.M.

AU - Steiner, M.

PY - 2005/7/25

Y1 - 2005/7/25

N2 - The Ni-58 (t, He-3)Co-58 reaction at 112 MeV/nucleon was measured to identify strength associated with Gamow-Teller transitions in the T-z = +1 direction. The experiment is a test case for future similar studies. The main aim of such studies is to test theoretical models used to predict Gamow-Teller strength distributions that serve as input for supernovae evolution calculations. The results indicate that the (t, He-3) reaction is indeed a powerful tool to perform such tests.

AB - The Ni-58 (t, He-3)Co-58 reaction at 112 MeV/nucleon was measured to identify strength associated with Gamow-Teller transitions in the T-z = +1 direction. The experiment is a test case for future similar studies. The main aim of such studies is to test theoretical models used to predict Gamow-Teller strength distributions that serve as input for supernovae evolution calculations. The results indicate that the (t, He-3) reaction is indeed a powerful tool to perform such tests.

KW - CHARGE-EXCHANGE REACTIONS

KW - SHELL-MODEL CALCULATIONS

KW - MASS RANGE A=45-65

KW - INTERACTION RATES

KW - DISTRIBUTIONS

KW - COLLAPSE

U2 - 10.1016/j.nuclphysa.2005.05.018

DO - 10.1016/j.nuclphysa.2005.05.018

M3 - Article

VL - 758

SP - 67C-70C

JO - Nuclear Physics A

JF - Nuclear Physics A

T2 - 8th International Symposium on Nucle in the Cosmos (NIC8)

Y2 - 19 July 2004 through 23 July 2004

ER -

Weak interaction strengths for supernovae calculations via the (t,3He) reaction on medium-heavy nuclei

Abstract

Keywords

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